Cross-correlation search for continuous gravitational waves from a compact object in SNR 1987A in LIGO Science Run 5
arXiv:1610.00059 · doi:10.1103/PhysRevD.94.082004
Abstract
We present the results of a cross-correlation search for gravitational waves from SNR 1987A using the second year of LIGO Science Run 5 data. The frequency band 75--450\,Hz is searched. No evidence of gravitational waves is found. A 90\% confidence upper limit of is placed on the gravitational wave strain at the most sensitive frequency near 150\,Hz. This corresponds to an ellipticity of and improves on previously published strain upper limits by a factor . We perform a comprehensive suite of validations of the search algorithm and identify several computational savings which marginally sacrifice sensitivity in order to streamline the parameter space being searched. We estimate detection thresholds and sensitivities through Monte-Carlo simulations.
References in corpus (10)
- LIGO: The Laser Interferometer Gravitational-Wave Observatory
- Searching for gravitational waves from Cassiopeia A with LIGO
- Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data
- New Phase-coherent Measurements of Pulsar Braking Indices
- The cross-correlation search for periodic gravitational waves
- First all-sky search for continuous gravitational waves from unknown sources in binary systems
- Gravitational waves from Sco X-1: A comparison of search methods and prospects for detection with advanced detectors
- Blandford's Argument: The Strongest Continuous Gravitational Wave Signal
- Model-Based Cross-Correlation Search for Gravitational Waves from Scorpius X-1
- F-statistic search for white-dwarf binaries in the first Mock LISA Data Challenge